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Non-Interacting New Agegraphic Dark Energy Model in f(Q) Gravity

2025/11/06 by M. Sharif, Madiha Ajmal, Sharif, M. +1
Physics and Astronomy · #Akaike information criterion #COSMIC cancer database #Chaplygin gas #Cosmology and Gravitation Theories #Dark energy #Equation of state #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #General Relativity and Quantum Cosmology (gr-qc) #Quintessence #Scale factor (cosmology) #Statistical Mechanics and Entropy

paper · pdf · doi:10.48550/arxiv.2511.04717

published in arXiv (Cornell University) (Cornell University)

openalex publication_date 2025/11/06 · openalex created_date 2025/11/11 · openalex updated_date 2026/08/05

Abstract

In this study, we explore the reconstruction of a new agegraphic dark energy model in a flat Friedmann-Robertson-Walker spacetime by f(Q) gravity framework, where Q represents non-metricity. We assume that the scale factor follows a power-law and explore how this model aligns with the expanding universe. In this perspective, we develop a new agegraphic f(Q) model and analyze the graphical behavior for cosmic evolution. We analyze physical characteristics of the model using the equation of state parameter, (ωDD) and the (r-s) planes. The equation of state parameter indicates a quintessence era characterized by accelerated expansion. The (ωDD)-plane identifies the freezing region and the Chaplygin gas model is represented in the (r-s)-plane. Finally, we examine the stability of the non-interacting model by evaluating the squared speed of sound. Our findings show that the non-interacting new agegraphic dark energy model effectively resolves the cosmic coincidence problem.

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